# Production Uncertainties of p-Nuclei in the γ-Process in Massive Stars Using a Monte Carlo Approach

@article{Rauscher2016ProductionUO,
title={Production Uncertainties of p-Nuclei in the $\gamma$-Process in Massive Stars Using a Monte Carlo Approach},
author={Thomas Rauscher and Nobuya Nishimura and Raphael Hirschi and Gabriele Cescutti and Alexander Murphy and Alexander Heger},
journal={arXiv: High Energy Astrophysical Phenomena},
year={2016},
volume={14},
pages={010509}
}
• Published 14 October 2016
• Materials Science
• arXiv: High Energy Astrophysical Phenomena
T. Rauscher, N. Nishimura, R. Hirschi, G. Cescutti, A. St J. Murphy and A. Heger, 'Production Uncertainties of p-Nuclei in the γ-Process in Massive Stars Using a Monte Carlo Approach', in Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016). Niigata, Japan, June 19-25, 2016. ISBN: 978-4-89027-118-4. DOI: http://dx.doi.org/10.7566/JPSCP.14.010509. © 2017 The Physical Society of Japan.

## References

SHOWING 1-10 OF 14 REFERENCES
Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations
• Physics
• 2016
T. Rauscher, N. Nishimura, R. Hirschi, G. Cescutti, A. St. J. Murphy and A. Heger, ‘Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations’, MNRAS Vol 463(
Sensitivity of p-process nucleosynthesis to nuclear reaction rates in a 25 M. supernova model
• Physics
• 2006
The astrophysical p-process, which is responsible for the origin of the proton-rich stable nuclei heavier than iron, was investigated using a full nuclear reaction network for a Type II supernova
Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data.
• Physics
Reports on progress in physics. Physical Society
• 2013
The main part of the review focuses on the nuclear uncertainties involved in the determination of the astrophysical reaction rates required for the extended reaction networks used in nucleosynthesis studies.
Theory Considerations For Nucleosynthesis Beyond Fe With Special Emphasis On p-Nuclei In Massive Stars
• Physics
• 2015
Nucleosynthesis of heavy elements requires the use of different experimental and theoretical methods to determine astrophysical reaction rates than light element nucleosynthesis. Additionally, there
COMPARED WITH VALUES IN PRIMITIVE METEORITES
• Physics
• 2014
The nucleosynthesis of proton-rich isotopes is calculated for multi-dimensional Chandrasekhar-mass models of Type Ia supernovae (SNe Ia) with different metallicities. The predicted abundances of the
Nucleosynthesis in massive stars with improved nuclear and stellar physics
• Physics
• 2002
We present the first calculations to follow the evolution of all stable nuclei and their radioactive progeni- tors in stellar models computed from the onset of central hydrogen burning through
NEUTRON CROSS SECTIONS FOR NUCLEOSYNTHESIS STUDIES
• Physics
• 2000
Previous compilations of (n, gamma) cross sections of relevance for neutron capture nucleosynthesis in the big bang and in the slow neutron capture process (s process) have been updated to encompass
Radiogenic p-isotopes from type Ia supernova, nuclear physics uncertainties, and galactic chemical evolution compared with values in primitive meteorites
• Physics
• 2014
The nucleosynthesis of proton-rich isotopes is calculated for multi-dimensional Chandrasekhar-mass models of Type Ia supernovae (SNe Ia) with different metallicities. The predicted abundances of the
Challenges in nucleosynthesis of trans-iron elements
Nucleosynthesis beyond Fe poses additional challenges not encountered when studying astrophysical processes involving light nuclei. Astrophysical sites and conditions are not well known for some of